Showing posts with label pyroxene. Show all posts
Showing posts with label pyroxene. Show all posts

Thursday, July 11, 2013

Horoman peridotite (lherzolite) - full thin section

 For a general description of the Horoman peridotite body, see the post of July 2, 2013: "Horoman Peridotite ... - olivine microfabfric".

This image shows a full thin section of Horoman peridotite. The 29-mm long dimension is actually shorter than a typical thin section, which is usually between 38 mm and 42 mm. The coarse texture of the peridotite is evident in this image. For example, the large olivine grain just left of center is about 10 mm in length. Most of the olivine grains are strained, as indicated by their banded coloration (deformation banding). The pyroxene grains also show deformation banding, but much less obviously than the olivine.

FULL THIN SECTION
Click on image to enlarge.          Photo © Daniel R. Snyder
Horoman peridotite (lherzolite), Hokkaido, Japan. Full thin section, XPL macrophotograph. Brightly-colored grains are olivine; gray grains are pyroxenes. Smaller, rounded brown grains are symplectite nodules. Imaged area approximately 21 mm by 29 mm.



REFERENCES

Niida,  K., (1975), Textures and Olivine Fabrics of the Horoman Ultramafic Rocks, Japan; Jour. Japan. Assoc. Min. Petr. Econ, Geol.; 70, p. 265-285. (In English with Japanese abstract)

Niida, K., (1984), Petrology of the Horoman Ultramafic Rocks in the Hidaka Metamorphic Belt, Hokkaido, Japan, Journal of the Faculty of Science, Hokkaido University. Series 4, Geology and mineralogy, 21(2):197-250. (In English)

Niida, K.,  and Takazawa, E. (2007), Origin of Layering observed in the Horoman Peridotite Complex, Japan, Jour. Geol Soc. Japan; 113:Supplement, p. 167-184. (In Japanese except for some of the figure labels)

Sawaguchi, T., (2004), Deformation history and exhumation process of the Horoman Peridotite Complex, Hokkaido, Japan. Tectonophysics, 379, p. 109-126. (In English)

Takahashi, N., (1991), Origin of three peridotite suites from the Horoman peridotite complex, Hokkaido, Japan; Melting, melt segregation, and solidification processes in the upper mantle; Jour. Min.Petr. Econ. Geol.,  86: p. 199-215. (In English) 


Friday, June 10, 2011

Pyroxene grains and pseudomorphs in Josephine serpentinized peridotite.

Click on image to enlarge.          Photo © Daniel R. Snyder
In this specimen,  A few very small remnants of olivine (bright-colored grains) can be seen around the image, but almost all of the olivine has been altered to serpentine. I collected this specimen on the border between the Josephine peridotite and the Onion Camp complex of Yule et al. (2006)*. I decided to call it Josephine peridotite for two reasons: 1. There is little evidence of shearing, and 2. Many large pyroxene grains still persist, and large serpentine pseudomorphs after pyroxene are distributed throughout the specimen. The large gray pyroxene grain at the left side of the image above still appears to be mostly pyroxene, while the broken grain in the center has been altered to bastite-texture serpentine. Hourglass-texture serpentine, probably an alteration product of olivine, occupies the rest of the image. Klamath Mountains, Josephine County, southwest Oregon, XPL. Imaged area 2.7 mm x 4 mm.

In the image below, the white spots on the large hand specimen are reflections from the surfaces of platy pseudomorphs after pyroxene; gray-green grains are pyroxene. Note that there appears to be more remnant pyroxene than pseudomorphosed pyroxene. The brown mesostatis is serpentine. The surface of the small hand specimen has been rough polished, showing dark grains of pyroxene. Lighter gray areas are serpentinized pyroxene grains (pseudomorphs). Scale is in centimeters.

Click on image to enlarge.          Photo © Daniel R. Snyder

*Yule, J. D., Saleeby, J. B., and Barnes, C. G., 2006, A rift-edge facies of the late Jurassic Rogue-Chetco arc and Josephine ophiolite, Klamath Mountains, Oregon, in Snoke, A. W. and Barnes, C.G., eds., Geological studies in the Klamath Mountain province, Californa and Oregon: A volume in honor of William P. Irwin: Geological Society of America Special Paper 410, p. 53-76.

Sunday, May 29, 2011

Presque Isle peridotite - full thin section

Click on image to enlarge.          Photo © Daniel R. Snyder
This image shows the texture of the peridotite, in which olivine and pyroxene have been almost entirely pseudomorphed by serpentine, much of which has been replaced in turn by amphiboles. Light-colored areas are carbonate veins. Marquette County, northern Michigan. XPL Macrophotograph. Imaged area 25 mm x 41 mm.

Wednesday, May 18, 2011

Talc in pyroxene in Webster dunite

Click on image to enlarge.          Photo © Daniel R. Snyder
A vein of talc (lower left to upper right) bisects two large grains of orthopyroxene, surrounded by olivine, in dunite. Webster-Addie ultramafic body, Blue Ridge Mountains, Jackson County, western North Carolina. XPL. Imaged area 2.7 mm x 4 mm.

Sunday, May 1, 2011

Pseudomorphs after pyroxene in ancient (1.2 Ga) metaperidotite

Click on the image to enlarge.      Sample: Jeff Chiarenzelli; Photo: Dan Snyder

A small body of highly-metamorphosed rocks jn the Adirondack lowlands has been interpreted as metaperidotite because of its CIPW normative mineralogy (harzburgite) and because pseudomorphs after ferromagnesian minerals have been found there (Chiarenzelli et al., 2011)*. The protolith has been dated at ~1.2 Ga using detrital zircons. In this image, two pseudomorphs after pyroxene, now probably consisting of an amphibole mineral, can be seen at left center and top center. Pyrites Complex, St. Lawrence County, northern New York. XPL. Imaged area 1.3 mm x 2 mm.

Thanks to Dr. Jeff Chiarenzelli, of St. Lawrence U., for the loan of this and many other thin sections.

* Jeff Chiarenzelli, Marian Lupulescu, Eric Thern, and Brian Cousens (2011), Tectonic implications of the discovery of a Shawinigan ophiolite (Pyrites Complex) in the Adirondack lowlasnds, Geosphere, 2011;7;333-356

Wednesday, April 13, 2011

Webster-Addie ultramafic body - sheared dunite, full thin section

Click on the image to enlarge. Click twice to enlarge more- it's a lot more 
interesting close up.      Photo: Dan Snyder.
Tectonized, sheared dunite. Upper 2/3 of image is composed mainly of polygonal olivine grains (more saturated colors) with scattered pyroxene grains (grays and pale yellows), especially at top left; lower 1/3 is composed of sheared talc clots with crushed and elongated grains of olivine and pyroxene. By itself, this thin section probably wouldn't fit the conventional definition of dunite - too much pyroxene - but it was part of a more extensive exposure that is clearly dunite. Webster-Addie ultramafic body, Blue Ridge Mountains, Jackson County, western North Carolina. XPL. Imaged area 22 mm x 39 mm.

Sunday, April 10, 2011

Pyroxene in dunite

Click on the image to enlarge.           Photo: Dan Snyder
A large orthopyroxene grain in dunite. According to the IUGS classification, a dunite is a rock made up of ferromagnesian minerals, mainly olivine and pyroxene, of which more than 90% is olivine (discounting accessory minerals). In practice, serpentine inferred to be derived from olivine is counted as olivine. Although a pyroxene grain dominates this photograph, there are only a few such grains in the sample.  Webster-Addie ultramafic body, Jackson County, North Carolina. Reflected-light photomicrograph of polished block. Ordinary light. Imaged area 3.3 mm x 4 mm.

Monday, April 4, 2011

Pyroxene lamellae, amphibole in dunite

Click on image to enlarge.           Photo: Dan Snyder

Exsolution lamellae in pyroxene (pale yellow grains at left and bottom, gray grain at right); ampohibole mineral (grains with diagonal cleavage patterns: center, top center); olivine (brightly colored grains at  center and top center). Webster-Addie utlramafic body, western North Carolina. XPL. Imaged area 1.3 mm x 2 mm.

Thanks to Dr. Michael Velbel, Michigan State U., for the loan of this and many other thin sections.

Saturday, March 5, 2011

Josephine peridotite (harzburgite) - Full thin section in cross-polarized light

Click on the image to enlarge. Copy the enlarged image to enlarge more - 
It looks much better close up.                      Photo © Daniel R. Snyder
Josephine peridotite, a component of the Josephine ophiolite sequence. Small, brightly colored grains are olivine, larger grains in shades of gray are orthopyroxene.  Josephine County, southwest Oregon. XPL macrophotograph of entire thin section. Imaged area 18 mm x 38 mm.

Wednesday, March 2, 2011

Josephine peridotite - digital mosaic

Ckick on image to enlarge.          Photo © Daniel R. Snyder
In this image: mostly olivine (bright colors) with incipient serpentinization, and a few large (gray) grains of orthopyroxene. Josephine peridotite, a component of the Josephine ophiolite sequence. Klamath Mountains, Josephine County, southwest Oregon. Digital mosaic of four 2x-objective images. XPL. Imaged area 5.1 mm x 7.6 mm.

Saturday, February 26, 2011

Josephine peridotite (harzburgite) - pyroxene

Click on image to enlarge.           Photo © Daniel R. Snyder
Josephine peridotite (partially serpentinized harzburgite), a component of the Josephine ophiolite sequence. Gray grain at left is pyroxene, large gray grain in center is partially serpentinized pyroxene (bastite texture). Brightly colored grains are olivine. Klamath Mountains, Josephine County, southwest Oregon.  XPL. Imaged area 1.3 mm x 2 mm.

Thursday, February 10, 2011

Presque Isle peridotite

Click on the image to enlarge.           Photo © Daniel R. Snyder
Peridotite (thoroughly serpentinized). Pseudomorphs of serpentine after olivine (dark green) and anthophyllite after pyroxenes (linear patterns of brown, orange, and yellow) retain the shapes of original crystals. I've seen the Presque Isle peridotite described as "highly deformed". This doesn't look highly deformed to me. A rock body whose protolith is a billion-plus years old and still preserves the original crystal shapes seems to me to hardly be deformed at all.

Michael Lewan's (1972)* M.S. thesis reports on three samples ranging from 54.9 percent to 59.2 percent serpentine by volume. Olivine plus augite account for another 15.7 to 21.2 percent total, about evenly divided. Lewan also found 4.4 percent to 7.8 percent anorthite in his three samples, but I've looked at several thin sections and haven't seen any. Presque Isle Park, City of Marquette, Marquette County, northern Michigan. XPL. Imaged area 1.3 x 2 mm. Link to photo of outcrop.

*Lewan, Michael D., 1972, Metasomatism and Weathering of the Presque Isle Serpentinized Peridotite, Marquette, Michigan, unpublished M.S. thesis, Michigan Technological University.

Sunday, February 6, 2011

Yellow Dog peridotite - clinopyroxene interstitial to olivine

Click on image to enlarge.          Photo © Daniel R. Snyder
The dark areas are olivine (partially serpentinized with stringers of magnetite), the magenta and violet shapes are clinopyroxene, and a few gray plagioclase laths show at the upper left. There appear to be several varieties of pyroxene in the Yellow Dog peridotite. One of the most noticeable is anhedral clinopyroxene occupying the interstices between fractured olivine crystals, as in this image. Apparently the pyroxene was the last major mineral to solidify from the melt (In his M.S. thesis, Morris (1977)* refers to these occurrences in the Yellow Dog peridotite as poikilitic texture). Also notice the dark rims around the olivine crystals, and the smooth interface between olivine and pyroxene, suggesting a reaction between the early-crystallizing olivine and the melt.  XPL. Imaged area 2.7 mm x 4 mm.

In the PPL enlargement (below) of the right center of the XPL image, the dark rims around the olivine appear to contain an iron-rich alteration product. The olivine fragments remaining in the core of the crystal are transparent in PPL. Imaged area of enlargement 1.3 mm x 2 mm.

Click on image to enlarge.          Photo © Daniel R. Snyder

Marquette County, northern Michigan.

*Morris, William J., (1977) Geochemistry and Origin of the Yellow Dog Plains Peridotite, Marquette County, Northern Michigan, unpublished master's thesis, Michigan state University.

Tuesday, January 18, 2011

Mantle lherzolite xenolith in basalt - full thin section.

Click on image to enlarge.           Photo © Daniel R. Snyder

Spinel lherzolite xenolith, San Carlos Indian Reservation, Arizona. Lherzolite is at left; brightly colored grains are olivine, gray and brown grains are pyroxene.  Felty-textured basalt is at right. XPL macrophotograph. Imaged area 21 mm x 34 mm. Click on the image to enlarge. It's a lot more interesting close up!

Monday, January 3, 2011

Mantle lherzolite xenolith in basalt - hand sample.

Click on image to enlarge.           Photo © Daniel R. Snyder
Granular lherzolite xenolith in basalt. Green masses are peridotite (lherzolite), gray mass is basalt. San Carlos Indian Reservation, Arizona. Scale in centimeters.

You probably know that peridotite is the commonest rock on the planet. Starting at the base of the crust and going straight down for 400 kilometers, the Earth's mantle is mostly peridotite as we know it at Earth-surface conditions.  Recall from petrology that there is compelling evidence for a phase change at the 400-km level. Because of the very high pressure at that that depth, olivine is thought to convert to a spinel structure - it's still olivine, (Mg,Fe)2SiO4, but it has a different crystal structure, and it's about 9 percent denser. This high-pressure polymorph of olivine undergoes another phase change at a depth of 670 kilometers. If that's all the peridotite there was, it would still represent 20 percent of the volume of Earth. Beyond the 670-km. level, and down to 2900 kilometers, everything is still mantle, and is believed to consist of other phase transformations of olivine, as well as pyroxenes and garnet, as pressure increases. So all in all the mantle, consisting mainly of peridotites (variously defined) accounts for 80 percent of the volume of our planet.

If you'd like to learn more about the composition and petrology of the mantle, most college petrology books devote a few pages to the subject. Beyond that,  I recommend a very thorough book by A. E. Ringwood, (1975), The Composition and Petrology of the Earth's Mantle, 604 p.,  McGraw-Hill. If your library doesn't have it, you can  get it used online for about $25.00. Ringwood later (1986) also wrote a shorter review of the subject in the Proceedings of the 4th International Kimberlite Conference, published by the Geological Society of Australia. It's only 29 pages and contains some updated references, and is an easier (and faster) read than the 1975 tome.

So, of there's so much peridotite on earth, why does so little of it crop out at the surface? As your petrology book will tell you, the short answer to that is that the rocks that form the upper crust are generated by partial melting of peridotite in the lower crust and upper mantle, which forms magma that works its way upward and solidifies as granites and other intrusive igneous rocks if it cools before it reaches the surface, or flows out on the surface as lavas that cool to form basalts and other extrusive igneous rocks. Since this is only partial melting, what remains behind in the mantle is still peridotite.

How do we know all this if we can't see into, or drill down or sink mineshafts into the mantle? A lot of what we know comes from indirect evidence - mainly seismic wave records, from which rock densities can be inferred. And in the past 50 years, great advances in experimental petrology have allowed scientists to replicate the behavior of rocks and minerals at mantle-like pressures. But in terms of looking at actual mantle-derived peridotites, there are only three ways this can be done. And again, these are listed in most petrology books:

1. Ultramafic xenoliths are carried to the surface by magma rising rapidly through conduits in mantle wall rock.  If a basaltic magma moves through peridotite country rock, it will pluck peridotite blocks from the wall of the conduit and carry them to the surface. Since the peridotite melts at a relatively high temperature, while the basaltic magma stays fluid at a lower temperature, the xenolith can reach the surface without being melted by the magma. The image above shows such a xenolith brought to the surface in an alkaline basalt. The deepest-origin xenoliths, from depths of more than 300 kilometers, are brought up in the magmas of kimberlites.

2. Because the oceanic crust is considerably thinner than the continental crust, mantle rocks are sometimes exposed on the ocean floor along fault zones. Of course, these are samples only of the uppermost mantle.

3. Ophiolites are layered mafic and ultramafic rock sequences, formerly oceanic crust and upper mantle, that were emplaced onto active continental margins. Sometimes transported far inland by low-angle thrust faulting, as in the Appalachians, the peridotite component of such an ophiolite survives as a coherent body of ultramafic rocks. The disadvantages of such ultramafic bodies are that they represent a sampling of only the shallowest part of the mantle, they are typically metamorphosed (recrystallized), so the original fabric and structure are destroyed, and they are highly susceptible to alteration into serpentine, talc, chlorite, and other hydrous secondary minerals. The advantage of these bodies - originally, and still, called Alpine peridotites - is that they are widely distributed throughout the world, and are generally accessible for study. Many of the images in the later pages of this blog are from such exposures.